QR Code

Debris disks around stars in the NIKA2 era

The new NIKA2 camera at the IRAM 30m radiotelescope was used to observe three known debris disks in order to constrain the SED of their dust emission in the millimeter wavelength domain. We have found that the spectral index between the two NIKA2 bands (1mm and 2mm) is consistent with the Rayleigh-J...

Whakaahuatanga katoa

I tiakina i:
Ngā kaituhi matua: Lestrade J.-F., Augereau J.-C., Booth M., Adam R., Ade P., André P., Andrianasolo A., Aussel H., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Holland W., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lefèvre C., Macías-Pérez J.F., Mauskopf P., Mayet F., Monfardini A., Perotto L., Pisano G., Ponthieu N., Revéret V., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Shu S., Sievers A., Thébault P., Tucker C., Zylka R.
Hōputu: Artigo
Reo:Inglês
I whakaputaina: EDP Sciences 2020-01-01
Rangatū:EPJ Web of Conferences
Urunga tuihono:https://www.epj-conferences.org/articles/epjconf/pdf/2020/04/epjconf_mmuniverse2019_00015.pdf
Ngā Tūtohu: Tāpirihia he Tūtohu
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!

Ngā tūemi rite